! Started logfile: J2258-2758_X_2017_03_27_pus_uvs.log on Sat Apr 27 22:09:18 2019 obs J2258-2758_X_2017_03_27_pus_uva.fits ! Reading UV FITS file: J2258-2758_X_2017_03_27_pus_uva.fits ! AN table 1: 32 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.728472 visibilities/baseline/integration-bin. ! Found source: J2258-2758 ! ! There are 12 IFs, and a total of 12 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.44388e+09 3.2e+07 1 3.2e+07 ! 02 2 8.47588e+09 3.2e+07 1 3.2e+07 ! 03 3 8.50788e+09 3.2e+07 1 3.2e+07 ! 04 4 8.53988e+09 3.2e+07 1 3.2e+07 ! 05 5 8.60388e+09 3.2e+07 1 3.2e+07 ! 06 6 8.63588e+09 3.2e+07 1 3.2e+07 ! 07 7 8.69988e+09 3.2e+07 1 3.2e+07 ! 08 8 8.73188e+09 3.2e+07 1 3.2e+07 ! 09 9 8.79588e+09 3.2e+07 1 3.2e+07 ! 10 10 8.82788e+09 3.2e+07 1 3.2e+07 ! 11 11 8.85988e+09 3.2e+07 1 3.2e+07 ! 12 12 8.89188e+09 3.2e+07 1 3.2e+07 ! ! Polarization(s): RR ! ! Read 1844 lines of history. ! ! Reading 12588 visibilities. select I ! Polarization I is unavailable. ! Selecting polarization: RR, channels: 1..12 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 ! Reading IF 5 channels: 5..5 ! Reading IF 6 channels: 6..6 ! Reading IF 7 channels: 7..7 ! Reading IF 8 channels: 8..8 ! Reading IF 9 channels: 9..9 ! Reading IF 10 channels: 10..10 ! Reading IF 11 channels: 11..11 ! Reading IF 12 channels: 12..12 print "field_size =",field_size ! field_size = 512 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J2258-2758_X_2017_03_27_pus] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 5. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 6. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 7. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 8. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 9. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 10. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 11. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 12. ! A total of 48 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.533067Jy sigma=0.003947 ! Fit after self-cal, rms=0.528711Jy sigma=0.003914 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.6572 mas, bmaj=1.694 mas, bpa=1.654 degrees ! Estimated noise=1317.61 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.0925 Jy ! Component: 100 - total flux cleaned = 1.36027 Jy ! Total flux subtracted in 100 components = 1.36027 Jy ! Clean residual min=-0.031615 max=0.101042 Jy/beam ! Clean residual mean=-0.000162 rms=0.009750 Jy/beam ! Combined flux in latest and established models = 1.36027 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 1.36027 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.252720Jy sigma=0.001769 ! Fit after self-cal, rms=0.252700Jy sigma=0.001769 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.103927 Jy ! Component: 100 - total flux cleaned = 0.160777 Jy ! Total flux subtracted in 100 components = 0.160777 Jy ! Clean residual min=-0.021893 max=0.038246 Jy/beam ! Clean residual mean=-0.000056 rms=0.005850 Jy/beam ! Combined flux in latest and established models = 1.52105 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 17 components and 1.52105 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.186108Jy sigma=0.001209 ! Fit after self-cal, rms=0.186014Jy sigma=0.001208 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Added new window around map position (-3.6, -4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0404681 Jy ! Component: 100 - total flux cleaned = 0.0693238 Jy ! Total flux subtracted in 100 components = 0.0693238 Jy ! Clean residual min=-0.019301 max=0.024198 Jy/beam ! Clean residual mean=-0.000024 rms=0.004918 Jy/beam ! Combined flux in latest and established models = 1.59037 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 34 components and 1.59037 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.171370Jy sigma=0.001084 ! Fit after self-cal, rms=0.171096Jy sigma=0.001081 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8597 mas, bmaj=2.151 mas, bpa=3.1 degrees ! Estimated noise=865.561 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-1.2, -2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0365561 Jy ! Component: 100 - total flux cleaned = 0.0592173 Jy ! Component: 150 - total flux cleaned = 0.0674288 Jy ! Component: 200 - total flux cleaned = 0.0713293 Jy ! Total flux subtracted in 200 components = 0.0713293 Jy ! Clean residual min=-0.016671 max=0.016513 Jy/beam ! Clean residual mean=0.000010 rms=0.004124 Jy/beam ! Combined flux in latest and established models = 1.6617 Jy ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 62 components and 1.6617 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.160583Jy sigma=0.001004 ! Fit after self-cal, rms=0.160105Jy sigma=0.000999 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.97 HN 1.42 KP 0.99 ! LA 1.00 MK 0.99 NL 1.01 OV 1.00 ! PT 0.99 SC 1.02 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.97 HN 1.36 KP 1.00 ! LA 1.00 MK 0.99 NL 1.01 OV 1.00 ! PT 0.98 SC 1.01 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.96 HN 1.28 KP 0.94 ! LA 1.03 MK 1.00 NL 1.00 OV 1.00 ! PT 0.98 SC 1.01 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.95 HN 1.35 KP 0.97 ! LA 1.03 MK 1.01 NL 1.01 OV 1.00 ! PT 0.99 SC 1.01 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.94 HN 1.25 KP 0.97 ! LA 1.02 MK 1.02 NL 0.99 OV 0.99 ! PT 0.99 SC 1.00 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.95 HN 1.34 KP 0.96 ! LA 1.02 MK 1.00 NL 1.00 OV 1.00 ! PT 0.98 SC 1.01 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.96 HN 1.29 KP 0.96 ! LA 1.04 MK 1.01 NL 1.00 OV 1.00 ! PT 0.98 SC 1.01 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.00 HN 1.32 KP 0.96 ! LA 1.01 MK 0.99 NL 1.00 OV 0.99 ! PT 0.98 SC 1.01 ! ! ! Correcting IF 9. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.96 HN 1.31 KP 0.96 ! LA 1.02 MK 0.98 NL 0.99 OV 0.99 ! PT 0.99 SC 0.97 ! ! ! Correcting IF 10. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 FD 0.95 HN 1.29 KP 0.86 ! LA 1.03 MK 0.99 NL 0.88 OV 1.08 ! PT 1.04 SC 0.94 ! ! ! Correcting IF 11. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.02 HN 1.42 KP 0.97 ! LA 1.09 MK 1.04 NL 0.94 OV 1.13 ! PT 1.13 SC 1.02 ! ! ! Correcting IF 12. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.97 HN 1.32 KP 0.99 ! LA 1.04 MK 0.98 NL 0.91 OV 1.10 ! PT 1.09 SC 1.00 ! ! ! Fit before self-cal, rms=0.160105Jy sigma=0.000999 ! Fit after self-cal, rms=0.113474Jy sigma=0.000713 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.863 mas, bmaj=2.153 mas, bpa=3.11 degrees ! Estimated noise=860.968 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00565976 Jy ! Component: 100 - total flux cleaned = 0.00611638 Jy ! Component: 150 - total flux cleaned = 0.00643108 Jy ! Component: 200 - total flux cleaned = 0.00683778 Jy ! Total flux subtracted in 200 components = 0.00683778 Jy ! Clean residual min=-0.006658 max=0.008559 Jy/beam ! Clean residual mean=-0.000000 rms=0.002088 Jy/beam ! Combined flux in latest and established models = 1.66854 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 79 components and 1.66854 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.112628Jy sigma=0.000707 ! Fit after self-cal, rms=0.112567Jy sigma=0.000706 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec selfcal true, true, soltime1 ! Performing amp+phase self-cal over 120 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.112567Jy sigma=0.000706 ! Fit after self-cal, rms=0.110062Jy sigma=0.000683 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8632 mas, bmaj=2.156 mas, bpa=3.16 degrees ! Estimated noise=860.992 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00477757 Jy ! Component: 100 - total flux cleaned = 0.00521696 Jy ! Component: 150 - total flux cleaned = 0.0053315 Jy ! Component: 200 - total flux cleaned = 0.00552724 Jy ! Total flux subtracted in 200 components = 0.00552724 Jy ! Clean residual min=-0.005483 max=0.005778 Jy/beam ! Clean residual mean=-0.000040 rms=0.001568 Jy/beam ! Combined flux in latest and established models = 1.67407 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 88 components and 1.67407 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.109651Jy sigma=0.000680 ! Fit after self-cal, rms=0.109641Jy sigma=0.000680 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000766235 Jy ! Component: 100 - total flux cleaned = 0.000858221 Jy ! Component: 150 - total flux cleaned = 0.000938235 Jy ! Component: 200 - total flux cleaned = 0.000862649 Jy ! Total flux subtracted in 200 components = 0.000862649 Jy ! Clean residual min=-0.005276 max=0.005749 Jy/beam ! Clean residual mean=-0.000038 rms=0.001539 Jy/beam ! Combined flux in latest and established models = 1.67493 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 93 components and 1.67493 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.109500Jy sigma=0.000679 ! Fit after self-cal, rms=0.109496Jy sigma=0.000679 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.109496Jy sigma=0.000679 ! Fit after self-cal, rms=0.105731Jy sigma=0.000645 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8631 mas, bmaj=2.157 mas, bpa=3.176 degrees ! Estimated noise=861.246 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00114992 Jy ! Component: 100 - total flux cleaned = 0.00132968 Jy ! Component: 150 - total flux cleaned = 0.00133393 Jy ! Component: 200 - total flux cleaned = 0.00119855 Jy ! Total flux subtracted in 200 components = 0.00119855 Jy ! Clean residual min=-0.003059 max=0.004563 Jy/beam ! Clean residual mean=0.000029 rms=0.000783 Jy/beam ! Combined flux in latest and established models = 1.67613 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 109 components and 1.67613 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.105614Jy sigma=0.000644 ! Fit after self-cal, rms=0.105614Jy sigma=0.000644 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-6, -3.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00394134 Jy ! Component: 100 - total flux cleaned = 0.00497414 Jy ! Component: 150 - total flux cleaned = 0.00504233 Jy ! Component: 200 - total flux cleaned = 0.00510677 Jy ! Total flux subtracted in 200 components = 0.00510677 Jy ! Clean residual min=-0.002799 max=0.002639 Jy/beam ! Clean residual mean=0.000031 rms=0.000704 Jy/beam ! Combined flux in latest and established models = 1.68123 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 125 components and 1.68123 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.105450Jy sigma=0.000643 ! Fit after self-cal, rms=0.105435Jy sigma=0.000643 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. win_mult = win_mult * 1.2 selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.105435Jy sigma=0.000643 ! Fit after self-cal, rms=0.105387Jy sigma=0.000643 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=2.436 mas, bmaj=5.777 mas, bpa=3.555 degrees ! Estimated noise=1091.92 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000808918 Jy ! Component: 100 - total flux cleaned = 0.00103261 Jy ! Component: 150 - total flux cleaned = 0.00126986 Jy ! Component: 200 - total flux cleaned = 0.00143353 Jy ! Total flux subtracted in 200 components = 0.00143353 Jy ! Clean residual min=-0.002343 max=0.003197 Jy/beam ! Clean residual mean=0.000061 rms=0.000851 Jy/beam ! Combined flux in latest and established models = 1.68267 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 139 components and 1.68267 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.105352Jy sigma=0.000642 ! Fit after self-cal, rms=0.105348Jy sigma=0.000642 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00013155 Jy ! Component: 100 - total flux cleaned = 0.000211997 Jy ! Component: 150 - total flux cleaned = 0.000349488 Jy ! Component: 200 - total flux cleaned = 0.00044166 Jy ! Total flux subtracted in 200 components = 0.00044166 Jy ! Clean residual min=-0.002305 max=0.003238 Jy/beam ! Clean residual mean=0.000062 rms=0.000845 Jy/beam ! Combined flux in latest and established models = 1.68311 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 143 components and 1.68311 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.105329Jy sigma=0.000642 ! Fit after self-cal, rms=0.105327Jy sigma=0.000642 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.863 mas, bmaj=2.157 mas, bpa=3.182 degrees ! Estimated noise=860.991 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.863 x 2.157 at 3.182 degrees (North through East) ! Clean map min=-0.004233 max=1.4461 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.105327Jy sigma=0.000642 ! Fit after self-cal, rms=0.099898Jy sigma=0.000598 ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8632 mas, bmaj=2.158 mas, bpa=3.194 degrees ! Estimated noise=860.919 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000117785 Jy ! Component: 100 - total flux cleaned = -0.000186082 Jy ! Component: 150 - total flux cleaned = -0.000240442 Jy ! Component: 200 - total flux cleaned = -0.000290685 Jy ! Total flux subtracted in 200 components = -0.000290685 Jy ! Clean residual min=-0.002613 max=0.002652 Jy/beam ! Clean residual mean=0.000030 rms=0.000649 Jy/beam ! Combined flux in latest and established models = 1.68282 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 149 components and 1.68282 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.099824Jy sigma=0.000598 ! Fit after self-cal, rms=0.099821Jy sigma=0.000598 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 4.92276e-05 Jy ! Component: 100 - total flux cleaned = 4.92808e-05 Jy ! Component: 150 - total flux cleaned = 2.26925e-06 Jy ! Component: 200 - total flux cleaned = -4.32445e-05 Jy ! Total flux subtracted in 200 components = -4.32445e-05 Jy ! Clean residual min=-0.002589 max=0.002643 Jy/beam ! Clean residual mean=0.000030 rms=0.000638 Jy/beam ! Combined flux in latest and established models = 1.68277 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 154 components and 1.68277 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.099777Jy sigma=0.000598 ! Fit after self-cal, rms=0.099776Jy sigma=0.000597 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.099776Jy sigma=0.000597 ! Fit after self-cal, rms=0.099748Jy sigma=0.000597 print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.6602 mas, bmaj=1.701 mas, bpa=1.808 degrees ! Estimated noise=1314.94 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.09014 Jy ! Component: 100 - total flux cleaned = 1.35355 Jy ! Component: 150 - total flux cleaned = 1.45428 Jy ! Component: 200 - total flux cleaned = 1.50883 Jy ! Total flux subtracted in 200 components = 1.50883 Jy ! Clean residual min=-0.010276 max=0.029078 Jy/beam ! Clean residual mean=-0.000081 rms=0.003731 Jy/beam ! Combined flux in latest and established models = 1.50883 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 21 model components to the UV plane model. ! The established model now contains 21 components and 1.50883 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8631 mas, bmaj=2.158 mas, bpa=3.199 degrees ! Estimated noise=860.763 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.05827 Jy ! Component: 100 - total flux cleaned = 0.0947372 Jy ! Component: 150 - total flux cleaned = 0.118736 Jy ! Component: 200 - total flux cleaned = 0.134689 Jy ! Total flux subtracted in 200 components = 0.134689 Jy ! Clean residual min=-0.004489 max=0.010826 Jy/beam ! Clean residual mean=-0.000012 rms=0.001607 Jy/beam ! Combined flux in latest and established models = 1.64352 Jy ! Adding 52 model components to the UV plane model. ! The established model now contains 63 components and 1.64352 Jy ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Added new window around map position (-4.4, -3.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0116753 Jy ! Component: 100 - total flux cleaned = 0.0195477 Jy ! Component: 150 - total flux cleaned = 0.0252668 Jy ! Component: 200 - total flux cleaned = 0.029182 Jy ! Total flux subtracted in 200 components = 0.029182 Jy ! Clean residual min=-0.002920 max=0.003617 Jy/beam ! Clean residual mean=0.000022 rms=0.000792 Jy/beam ! Combined flux in latest and established models = 1.6727 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 90 components and 1.6727 Jy ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Added new window around map position (-2.8, -3.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00285259 Jy ! Component: 100 - total flux cleaned = 0.0045184 Jy ! Component: 150 - total flux cleaned = 0.00612725 Jy ! Component: 200 - total flux cleaned = 0.00700309 Jy ! Total flux subtracted in 200 components = 0.00700309 Jy ! Clean residual min=-0.002619 max=0.002934 Jy/beam ! Clean residual mean=0.000029 rms=0.000671 Jy/beam ! Combined flux in latest and established models = 1.6797 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 108 components and 1.6797 Jy ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Added new window around map position (-23, 18.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00161616 Jy ! Component: 100 - total flux cleaned = 0.00224487 Jy ! Component: 150 - total flux cleaned = 0.00259924 Jy ! Component: 200 - total flux cleaned = 0.00299377 Jy ! Total flux subtracted in 200 components = 0.00299377 Jy ! Clean residual min=-0.002438 max=0.002373 Jy/beam ! Clean residual mean=0.000024 rms=0.000615 Jy/beam ! Combined flux in latest and established models = 1.6827 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 117 components and 1.6827 Jy ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=2.436 mas, bmaj=5.775 mas, bpa=3.559 degrees ! Estimated noise=1091.65 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00184781 Jy ! Component: 100 - total flux cleaned = 0.00244078 Jy ! Component: 150 - total flux cleaned = 0.00293511 Jy ! Component: 200 - total flux cleaned = 0.00307968 Jy ! Total flux subtracted in 200 components = 0.00307968 Jy ! Clean residual min=-0.001950 max=0.002656 Jy/beam ! Clean residual mean=0.000050 rms=0.000737 Jy/beam ! Combined flux in latest and established models = 1.68578 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 5.10635e-05 Jy ! Component: 100 - total flux cleaned = 5.20326e-05 Jy ! Component: 150 - total flux cleaned = 9.66257e-06 Jy ! Component: 200 - total flux cleaned = -1.09138e-05 Jy ! Total flux subtracted in 200 components = -1.09138e-05 Jy ! Clean residual min=-0.001944 max=0.002651 Jy/beam ! Clean residual mean=0.000050 rms=0.000731 Jy/beam ! Combined flux in latest and established models = 1.68577 Jy ! Adding 34 model components to the UV plane model. ! The established model now contains 141 components and 1.68577 Jy ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8631 mas, bmaj=2.158 mas, bpa=3.199 degrees ! Estimated noise=860.763 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000717215 Jy ! Component: 100 - total flux cleaned = -0.000822804 Jy ! Component: 150 - total flux cleaned = -0.000820806 Jy ! Component: 200 - total flux cleaned = -0.000914411 Jy ! Total flux subtracted in 200 components = -0.000914411 Jy ! Clean residual min=-0.002324 max=0.002453 Jy/beam ! Clean residual mean=0.000025 rms=0.000585 Jy/beam ! Combined flux in latest and established models = 1.68485 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 151 components and 1.68485 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.099571Jy sigma=0.000597 ! Fit after self-cal, rms=0.099557Jy sigma=0.000597 wmodel J2258-2758_X_2017_03_27_pus_map.mod ! Writing 151 model components to file: J2258-2758_X_2017_03_27_pus_map.mod wobs J2258-2758_X_2017_03_27_pus_uvs.fits ! Writing UV FITS file: J2258-2758_X_2017_03_27_pus_uvs.fits wwins J2258-2758_X_2017_03_27_pus_map.win ! wwins: Wrote 7 windows to J2258-2758_X_2017_03_27_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00041172 Jy ! Component: 100 - total flux cleaned = 0.000655228 Jy ! Component: 150 - total flux cleaned = 0.000730903 Jy ! Component: 200 - total flux cleaned = 0.000765375 Jy ! Component: 250 - total flux cleaned = 0.000868449 Jy ! Component: 300 - total flux cleaned = 0.00106718 Jy ! Component: 350 - total flux cleaned = 0.00119647 Jy ! Component: 400 - total flux cleaned = 0.00119716 Jy ! Component: 450 - total flux cleaned = 0.0013207 Jy ! Component: 500 - total flux cleaned = 0.00132039 Jy ! Component: 550 - total flux cleaned = 0.00134991 Jy ! Component: 600 - total flux cleaned = 0.00137892 Jy ! Component: 650 - total flux cleaned = 0.00140749 Jy ! Component: 700 - total flux cleaned = 0.00143602 Jy ! Component: 750 - total flux cleaned = 0.00146395 Jy ! Component: 800 - total flux cleaned = 0.00154521 Jy ! Component: 850 - total flux cleaned = 0.0016249 Jy ! Component: 900 - total flux cleaned = 0.00159824 Jy ! Component: 950 - total flux cleaned = 0.00162422 Jy ! Component: 1000 - total flux cleaned = 0.00167502 Jy ! Component: 1050 - total flux cleaned = 0.00172537 Jy ! Component: 1100 - total flux cleaned = 0.00177503 Jy ! Component: 1150 - total flux cleaned = 0.00179961 Jy ! Component: 1200 - total flux cleaned = 0.00177578 Jy ! Component: 1250 - total flux cleaned = 0.00187229 Jy ! Component: 1300 - total flux cleaned = 0.00194361 Jy ! Component: 1350 - total flux cleaned = 0.00191984 Jy ! Component: 1400 - total flux cleaned = 0.00196661 Jy ! Component: 1450 - total flux cleaned = 0.00196672 Jy ! Component: 1500 - total flux cleaned = 0.00201191 Jy ! Component: 1550 - total flux cleaned = 0.00201187 Jy ! Component: 1600 - total flux cleaned = 0.0020119 Jy ! Component: 1650 - total flux cleaned = 0.00201205 Jy ! Component: 1700 - total flux cleaned = 0.00205605 Jy ! Component: 1750 - total flux cleaned = 0.0020343 Jy ! Component: 1800 - total flux cleaned = 0.00203406 Jy ! Component: 1850 - total flux cleaned = 0.0020342 Jy ! Component: 1900 - total flux cleaned = 0.00203407 Jy ! Component: 1950 - total flux cleaned = 0.00209638 Jy ! Component: 2000 - total flux cleaned = 0.00203429 Jy ! Total flux subtracted in 2048 components = 0.00209579 Jy ! Clean residual min=-0.001087 max=0.001212 Jy/beam ! Clean residual mean=0.000015 rms=0.000384 Jy/beam ! Combined flux in latest and established models = 1.68695 Jy keep ! Adding 153 model components to the UV plane model. ! The established model now contains 304 components and 1.68695 Jy ![Exited script file: muppet] wmap "J2258-2758_X_2017_03_27_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8631 x 2.158 at 3.199 degrees (North through East) ! Clean map min=-0.0034641 max=1.4435 Jy/beam ! Writing clean map to FITS file: J2258-2758_X_2017_03_27_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.44354 invert ! Inverting map ! Your choice of large map pixels excluded 0.111% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000383197 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0796367 0.0796367 0.159273 0.318547 0.637094 1.27419 2.54837 5.09675 10.1935 20.387 40.774 81.548 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0011 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.443 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8631 x 2.158 at 3.199 degrees (North through East) ! Clean map min=-0.0034641 max=1.4435 Jy/beam ! Error occured in command: mapplot ! ! ! ! ! ! 4 consecutive EOF's on stdin - 10 will exit program ! ! 5 consecutive EOF's on stdin - 10 will exit program ! ! 6 consecutive EOF's on stdin - 10 will exit program ! ! 7 consecutive EOF's on stdin - 10 will exit program ! ! 8 consecutive EOF's on stdin - 10 will exit program ! ! 9 consecutive EOF's on stdin - 10 will exit program ! ! 10 consecutive EOF's on stdin - 10 will exit program ! Log file J2258-2758_X_2017_03_27_pus_uvs.log closed on Sat Apr 27 22:09:19 2019